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Fig. B.1.

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Arm/interarm contrast in SFR surface density based on extinction-corrected Hα from MUSE as a function of the SFR contrast inferred directly from Hα (without accounting for extinction). Open circles represent radial measurements (in radial bins of 500 pc) across all PHANGS–MUSE galaxies, while orange circles show the mean contrast for each spiral segment (typically contributing two points per galaxy).

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